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임계 레이놀즈 수 이하에서 웨이비핀의 각도에 따른 크로스 컷팅이 압력강하에 미치는 영향 분석

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(1)

초 록

   



figure 1. 수치해석 대상의 Geometry

(2)

  

 

 

 

 

 

 

 

 

  ∂ 

∂ 

 

∂ ∂ 

figure 2. Simulation Geometry

figure 4. Re=400, Grid Dependency Test figure 3. Grids for Near Wall

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  

   



  

  

 

Mesh Number friction factor Std.(%)

9600 0.1352339

21600 0.1191462 11.896206

29400 0.1153004 3.2278184

38400 0.1127767 2.1888027

48600 0.1110525 1.5287985

86400 0.1101612 0.8026134

figure 5. Grid Dependency Test: Std 비교

Space Ratio   °   °   °

0.15 above 510 510 340

figure 7. Corrugation Angle 별 임계 레이놀즈 수 (Comini et al.[3])

200 400 600 800 1000

0.05 0.1 0.15 0.2 0.25 0.3 0.35

Ali & Ramadhyani PRESENT

f

Re

figure 6. Ali & Ramadhyani의 실험값과의 validation

(4)

10 20 30 0.14

0.21

Angle

NOCUT CUT

f factor

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



(6)

W. M. Kays, A. L. London, 1984, “Compact Heat Exchangers, 3rd”, ed. Mcgraw-Hill, New-York

M. M. Ali and S. Ramadhyani, 1992, “Experiments on convective heat transfer in corrugated channels”, Experimental Heat Transfer, vol. 5, pp.175-193

G. Comini, C. Nonino and S. Savino, 2002, “Convective heat and mass transfer in wavy finned-tube exchangers”, international journal of numberical methods for heat & fluid flow, vol. 12 Iss 6, pp 735-755

G. Comini, C. Nonino and S. Savino, 2002, “Effect of space ratio and corrugation angle on convection enhancement in wavy channels”, international journal of numberical methods for heat

& fluid flow, vol. 13 Iss 4, pp 500-519

M. Manglik and E. Bergles., 1995, “Heat Trasnfer and Pressure Drop Correlations for the Rectangular Offset Strip Fin Compact Heat Exchanger”, Exp. Therm. Fluid Sci. 10(2), 171-180 Tae Young Kim. and Sung Jin, Kim., 2009, “Fluid flow and

heat transfer characteristic of cross-cut heat sinks”, International Journal of Heat and Mass Transfer; 52, pp. 5358-5370

수치

figure  1.  수치해석  대상의  Geometry
figure  4.  Re=400,  Grid  Dependency  Testfigure  3.  Grids  for  Near  Wall
figure  7.  Corrugation  Angle  별  임계  레이놀즈  수  (Comini  et  al.[3])

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